Note on the dependence of Pc3-4 activity on the solar wind velocity

Details Note on the dependence of Pc3-4 activity on the solar wind velocity Note on the dependence of Pc3-4 activity on the solar wind velocity

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994angeo..12.1192g&link_type=abstract

Annales Geophysicae (ISSN 0992-7689), vol. 12, no. 12, p. 1192-1196

Mathematics

Logic

3

Amplitudes, Earth Magnetosphere, Mathematical Models, Solar Wind, Solar Wind Velocity, Correlation Coefficients, Protons, Proving, Shock Waves

Scientific paper

Various models that describe the dependence of pulsation amplitude A on the solar wind velocity V are discussed. Phenomenological considerations and experimental data count in favor of a model of the form A/A0 = (V/V0) exp (-V0/V). The linear model A = a + bV which is common in the literature gives negative values of amplitudes as V approaches 0, which is strange from the physical point of view. The possibility of modifying the linear model by including critical phenomena is discussed.

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